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Semrock Master Catalog 2018

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Edge Steepness and Transition Width<br />

<strong>Semrock</strong> edge filters – including our steepest RazorEdge ® Raman filters as<br />

well as our EdgeBasic filters for application-specific Raman systems and<br />

fluorescence imaging – are specified with a guaranteed “Transition Width.”<br />

Transition Width = maximum allowed spectral width between the laser line<br />

(where OD > 6) and the 50% transmission point<br />

Any given filter can also be described by its “Edge Steepness,” which is the<br />

actual steepness of the filter, regardless of the precise wavelength placement<br />

of the edge.<br />

Edge Steepness = actual steepness of a filter measured<br />

from the OD 6 point to the 50% transmission point<br />

Figure 1 illustrates Transition Width and Edge Steepness for an edge<br />

filter designed to block the 785 nm laser line (example shows a U-grade<br />

RazorEdge filter). Table 1 below lists the guaranteed Transition Width and<br />

typical Edge Steepness (for 25 mm diameter parts) for <strong>Semrock</strong> edge filters.<br />

All RazorEdge filters provide exceptional steepness to allow measurement<br />

of signals very close to the blocked laser line with high signal-to-noise ratio.<br />

However, the state-of-the-art E-grade RazorEdge filters take closeness to<br />

an Extreme level.<br />

The graph at the right illustrates that U-grade RazorEdge filters have a<br />

transition width that is 1% of the laser wavelength. E-grade filters have a<br />

Transition width that is twice as narrow, or 0.5% of the laser line!<br />

Table 1<br />

PRODUCT NOTE<br />

Edge Filter Type<br />

TECHNICAL NOTE<br />

Guaranteed Transition<br />

Width<br />

(% of laser wavelength)<br />

Ultraviolet (UV) Raman Spectroscopy<br />

Raman spectroscopy measurements generally face two<br />

limitations: (1) Raman scattering cross sections are tiny,<br />

requiring intense lasers and sensitive detection systems just<br />

to achieve enough signal; and (2) the signal-to-noise ratio is<br />

further limited by fundamental, intrinsic noise sources like<br />

sample autofluorescence. Raman measurements are most<br />

commonly performed with green, red, or near-infrared (IR)<br />

lasers, largely because of the availability of established lasers<br />

and detectors at these wavelengths. However, by measuring<br />

Raman spectra in the ultraviolet (UV) wavelength range, both<br />

of the above limitations can be substantially alleviated.<br />

Visible and near-IR lasers have photon energies below the<br />

first electronic transitions of most molecules. However, when<br />

the photon energy of the laser lies within the electronic<br />

spectrum of a molecule, as is the case for UV lasers and<br />

most molecules, the intensity of Raman-active vibrations can<br />

increase by many orders of magnitude – this effect is called<br />

“resonance-enhanced Raman scattering.”<br />

Although UV lasers tend to excite strong autofluorescence,<br />

it typically occurs only at wavelengths above about 300 nm,<br />

Typical Edge<br />

Steepness<br />

(% of laser wavelength)<br />

RazorEdge E-grade < 0.5% (< 90 cm -1 for 532) 0.2% (1.1 nm for 532)<br />

RazorEdge U-grade < 1.0% (< 186 cm -1 for 532) 0.5% (2.7 nm for 532)<br />

EdgeBasic < 2.5% (< 458 cm -1 for 532) 1.5% (8.0 nm for 532)<br />

* except UV filters<br />

Signal<br />

Laser<br />

Line<br />

Transmission (% and OD)<br />

100%<br />

50%<br />

10%<br />

OD 1<br />

OD 2<br />

OD 3<br />

OD 4<br />

OD 5<br />

OD 6<br />

780 785 790<br />

795 800<br />

Raman<br />

Signal<br />

Laser<br />

Line<br />

Transition<br />

Width<br />

Edge<br />

Steepness<br />

Wavelength (nm)<br />

Figure 1: Transition width and edge steepness illustrated.<br />

Transmission (% and OD)<br />

80 0 -80<br />

-160 -240<br />

100%<br />

50%<br />

10%<br />

OD 1<br />

OD 2<br />

OD 3<br />

OD 4<br />

OD 5<br />

Wavenumber Shift from 785 nm (cm –1 )<br />

E-grade<br />

~ 0.2%<br />

U-grade<br />

0.5% 1.0%<br />

~ 0.5%<br />

OD 6<br />

780 785 790<br />

795 800<br />

Wavelength (nm)<br />

Figure 2: Transition widths and edge steepnesses for<br />

LP02-785RE and LP02-785RU filters (see page 94).<br />

Autofluorescence<br />

Noise<br />

200 225 250 275 300 325 350 375 400<br />

Wavelength (nm)<br />

independent of the UV laser wavelength. Since even<br />

a 4000 cm –1<br />

(very large) Stokes shift leads to Raman<br />

emission below 300 nm when excited by a common 266<br />

nm laser, autofluorescence simply does not interfere<br />

with the Raman signal making high signal-to-noise ratio<br />

measurements possible.<br />

An increasing number of compact, affordable, and highpower<br />

UV lasers have become widely available, such as<br />

quadrupled, diode-pumped Nd:YAG lasers at 266 nm<br />

and NeCu hollow-cathode metal-ion lasers at 248.6 nm,<br />

making ultra-sensitive UV Raman spectroscopy a now<br />

widely accessible technique.<br />

NIR Filters Mirrors Polarizers<br />

Edge<br />

Filters<br />

Dichroic<br />

Beamsplitters<br />

Laser-line<br />

Filters<br />

Laser Diode<br />

Filters<br />

Notch<br />

Filters<br />

Lamp Clean-up<br />

Filters<br />

93<br />

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